威尔金森微波各向异性小组运用计算机程序去发现产生声谱的微波大小的比例，正象棱镜转换波长到颜色。
The WMAP team used computer programs to find the proportion of wave sizes generating the sound spectrum, just as a prism converts light wavelengths to color.
在2003年，美国航空航天局的威尔金森微波各向异性探测器绘制出了一幅空前详细的早期微波天空的地图，也是第一张完整的地图。
In 2003 NASA's Wilkinson microwave Anisotropy Probe produced the first full map of the early microwave sky in unprecedented detail.
从威尔金森微波各向异性探测器(WMAP)得来的数据显示出，细微温度变化是在宇宙微波背景辐射移动通过银河星系团气体时产生的。
Data from the Wilkinson microwave Anisotropy Probe (WMAP) can show the minute temperature changes created as the cosmic microwave background radiation moves through gases in galaxy clusters.
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